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Table 4:

Dispersion of proper motions for each open cluster studied.
Cluster $N_{*{\rm s}}$ $\sigma_{\mu_{\alpha}\cos\delta}$ $\sigma_{\delta}$ $V_{\rm range}$

ALESSI 21
59 2.4 2.6 9.8-12.6
ASCC 24 13 2.1 3.4 7.5-11.7
ASCC 27 13 2.6 2.1 8.8-12.1
ASCC 30 33 1.5 1.8 8.9-12.2
BOCHUM 3 5 1.5 0.7 11.9-13.7
NGC 2184 8 2.6 2.1 9.6-12.2
NGC 2215 9 0.8 0.9 10.6-12.9
NGC 2232 9 1.2 2.3 7.8-10.6
NGC 2286 31 2.4 2.0 9.7-14.3
NGC 2302 20 0.8 2.1 10.8-12.5
NGC 2306 11 1.4 2.3 10.1-12.5
NGC 2311 14 1.4 1.4 10.2-12.6
NGC 2323 126 1.1 1.3 8.9-13.6
NGC 2335 8 2.1 1.1 10.7-12.7
NGC 2548 86 1.1 1.4 8.5-15.6

Number of stars and magnitude range is also given.


Source LaTeX | All tables | In the text

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